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Ricci Reheating

We present a model for viable gravitational reheating involving a scalar field directly coupled to the Ricci curvature scalar. Crucial to the model is a period of kination after inflation, which causes the Ricci scalar to change sign thus inducing a tachyonic effective mass m2  −H2 for the scalar fi...

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Bibliografski detalji
Glavni autori: Opferkuch, Toby, Schwaller, Pedro, Stefanek, Ben A.
Jezik:eng
Izdano: 2019
Teme:
Online pristup:https://dx.doi.org/10.1088/1475-7516/2019/07/016
http://cds.cern.ch/record/2674985